Quasinormal modes of Regular Black Hole Charge

Research paper by L. A. Lopez, Valeria Hinojosa

Indexed on: 21 Oct '18Published on: 21 Oct '18Published in: arXiv - General Relativity and Quantum Cosmology


The quasinormal modes (QNMs) of a regular black hole with charge are calculated in the eikonal approximation. In the eikonal limit the QNMs of black hole are determined by the parameters of the unstable circular null geodesics. The behaviors of QNMs are compared with QNMs of Reisner-Nordstr\"{o}m black hole, it is done by fixing some of the parameters that characterize the black holes and varying another. We observed that the parameter that is related one effective cosmological constant at small distances , determines the behaviors of the QNMs of regular black hole with charge.